| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.84 | 36.21 | 11.02 | 28.57 | -21.04 | 311.80 | -43.40 | 124.55 | 0.7801 | -105.1 | -15.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.33 | 2.22 | 0.99 | 1.65 | -20.79 | 315.08 | -40.12 | 126.22 | 0.7491 | 759.3 | 602.1 | |
| 0.00 | 0.80 | 0.00 | 0.60 | -21.12 | 314.76 | -40.44 | 126.40 | 0.7540 | 354.0 | 347.0 | |
| 0.00 | 1.51 | 0.00 | 1.13 | -20.93 | 314.61 | -40.59 | 126.08 | 0.7543 | 753.0 | 589.7 | |
| 1.24 | 2.40 | 0.93 | 1.80 | -20.64 | 314.45 | -40.75 | 125.65 | 0.7541 | 701.5 | 567.3 | |
| 0.00 | 0.27 | 0.00 | 0.20 | -20.89 | 314.19 | -41.01 | 125.78 | 0.7579 | 315.0 | 253.3 | |
| 1.86 | 7.01 | 1.41 | 5.30 | -20.57 | 314.00 | -41.20 | 125.30 | 0.7579 | 589.0 | 397.3 | |
| 0.00 | 0.44 | 0.00 | 0.34 | -20.31 | 312.84 | -42.37 | 124.28 | 0.7671 | 474.0 | 449.4 | |
| 0.00 | 1.51 | 0.00 | 1.17 | -20.33 | 312.57 | -42.64 | 124.15 | 0.7697 | 545.0 | 391.9 | |
| 0.00 | 1.42 | 0.00 | 1.15 | -21.57 | 310.81 | -44.39 | 124.54 | 0.7919 | -605.0 | -481.9 | |
| 0.53 | 3.64 | 0.43 | 2.96 | -21.42 | 310.23 | -44.97 | 124.05 | 0.7962 | -725.7 | -558.7 | |
| 0.00 | 0.44 | 0.00 | 0.36 | -20.69 | 310.42 | -44.78 | 123.34 | 0.7910 | -701.0 | -676.0 | |
| 4.79 | 12.60 | 3.93 | 10.33 | -21.52 | 309.87 | -45.33 | 123.96 | 0.7999 | -571.0 | -406.5 | |
| 0.98 | 1.95 | 0.79 | 1.58 | -20.78 | 310.16 | -45.04 | 123.30 | 0.7937 | -667.0 | -599.8 | |
| 3.11 | -12.00 | 2.54 | -12.00 | -21.17 | 309.96 | -45.24 | 123.62 | 0.7974 | -614.3 | 999999 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |